INTRODUCTION
A growing interest in the laser ion sources (LIS) in recent years has been based on their ability to produce ions with a broad spectrum of charge states (even higher than 50+) and with the kinetic energy in the MeV range. Moreover, they give extremely high ion current densities, which may attain values of hundreds of mA/cm2 in the far expansion zone (~1 m) (Haseroth & Hora, Reference Haseroth and Hora1996; Wolowski et al., Reference Wolowski, Badziak, Boody, Czarnecka, Gammino, Jablonski, Krása, Láska, Parys, Rohlena, Rosinski, Ryc, Torrisi and Ullschmied2006, Reference Wolowski, Badziak, Czarnecka, Parys, Pisarek, Rosinski, Turan and Yerci2007; Badziak, Reference Badziak2007). There are various factors that influence characteristics and amount of emitted ions more or less (Láska et al., Reference Láska, Badziak, Boody, Gammino, Jungwirth, Krása, Krouský, Parys, Pfeifer, Rohlena, Ryć, Skála, Torrisi, Ullschmied and Wolowski2007a, Reference Láska, Badziak, Boody, Gammino, Jungwirth, Krása, Krouský, Parys, Pfeifer, Rohlena, Ryć, Skála, Torrisi, Ullschmied and Wolowski2007b). These are the laser wavelength, the laser intensity, the focus setting, the angle of target irradiation, and the target surface properties. Very important is the focus position (FP) with regard to the target surface, because it determines not only the nominal laser intensity due to the caustic of the focused laser beam, but also the length- and time-scale of the interaction of the laser pulse with the preformed plasma (Láska et al., Reference Láska, Jungwirth, Králiková, Krása, Pfeifer, Rohlena, Skála, Ullschmied, Badziak, Parys, Wolowski, Woryna, Torrisi, Gammino and Boody2004a, Reference Láska, Badziak, Boody, Gammino, Jungwirth, Krása, Krouský, Parys, Pfeifer, Rohlena, Ryć, Skála, Torrisi, Ullschmied and Wolowski2007a).
At intensities above ~1 × 1014 W/cm2, the optimum FP makes the interaction of the laser radiation with the expanding plasma plume very effective and the conditions for occurrence of various non-linear processes (including ponderomotive and/or relativistic self-focusing (Hora,Reference Hora1969, 1975; Hauser et al., Reference Hauser, Scheid and Hora1992; Kumar et al., Reference Kumar, Gupta and Sharma2006; Láska et al., Reference Láska, Jungwirth, Krása, Krouský, Pfeifer, Rohlena, Skála, Ullschmied, Velyhan, Kubeš, Badziak, Parys, Rosinski, Ryc and Wolowski2006; Rowlands, Reference Rowlands2006)) can be met. Then heavy ions with the highest charge states and energy can be generated (Láska et al., Reference Láska, Badziak, Boody, Gammino, Hora, Jungwirth, Krása, Parys, Pfeifer, Rohlena, Torrisi, Ullschmid, Wolowski and Woryna2003, Reference Láska, Jungwirth, Krása, Pfeifer, Rohlena, Ullschmied, Badziak, Parys, Wolowski, Boody, Gammino and Torrisi2004b, Reference Láska, Jungwirth, Krása, Pfeifer, Rohlena, Ullschmied, Badziak, Parys, Wolowski, Gammino, Torrisi and Boody2005a). The necessary pre-formed plasma can be produced either by a suitable pre-pulse, preceding the main laser pulse, or due to the interaction of the front part of a sufficiently long main pulse (>100 ps), the rest of which interacts with the self-created plasma. Considering that ion generation starts at a laser intensity of ~109 W/cm2, short (i.e., ps and sub-ps) laser pulses interact with the pre-formed plasma, too, because of their much longer (nanosecond) background. Moreover, the intensity contrast of the main pulse related to that background is usually not good enough (Rus et al., Reference Rus, Zeitoun, Mocek, Sebban, Kalal, Demir, Jamelot, Klisnick, Kralikova, Skala and Tallents1997; Láska et al., Reference Láska, Jungwirth, Králiková, Krása, Pfeifer, Rohlena, Skála, Ullschmied, Gammino, Torrisi, Boody, Badziak, Parys, Wolowski and Woryna2002a, Reference Láska, Jungwirth, Králiková, Krása, Pfeifer, Rohlena, Skála, Ullschmied, Badziak, Parys, Wolowski, Woryna, Torrisi, Gammino and Boody2004a, Reference Láska, Jungwirth, Krása, Pfeifer, Rohlena and Ullschmied2005b, Reference Láska, Badziak, Boody, Gammino, Jungwirth, Krása, Krouský, Parys, Pfeifer, Rohlena, Ryć, Skála, Torrisi, Ullschmied and Wolowski2007a; Badziak et al., Reference Badziak, Kasperczuk, Parys, Pisarczyk, Rosinski, Ryć, Wolowski, Jablonski, Suchanska, Krouský, Láska, Mašek, Pfeifer, Ullschmied, Dareshwar, Foldes, Torrisi and Pisarczyk2007). The essence of the optimum position of the focus in front of the target surface has already been found (Láska et al., Reference Láska, Mašek, Králiková, Krása, Skála, Rohlena, Woryna, Wolowski, Langbein and Haseroth1994; Woryna et al., Reference Woryna, Parys, Wolowski, Láska, Krása, Mašek, Pfeifer, Králiková, Skála, Straka and Rohlena1996a), various asymmetric dependencies with regard to the position of nominal maximum laser intensity, observed later (Láska et al., Reference Láska, Ryc, Badziak, Boody, Gammino, Jungwirth, Krasa, Krousky, Mezzasalma, Parys, Pfeifer, Rohlena, Torrisi, Ullschmied and Wolowski2005c, Reference Láska, Badziak, Boody, Gammino, Jungwirth, Krása, Krouský, Parys, Pfeifer, Rohlena, Ryć, Skála, Torrisi, Ullschmied and Wolowski2007a; Kasperczuk et al., Reference Kasperczuk, Pisarczyk, Kalal, Martinková, Ullschmied, Krousky, Masek, Pfeifer, Rohlena, Skala and Pisarczyk2008), as well as the step in the dependence (Gitomer et al., Reference Gitomer, Jones, Begay, Ehler, Kepphart and Kristal1986, Fig. 4) can also be explained taking into account the interaction of the laser beam with the pre-formed plasma.
A lot of work has been invested on this topic, however, “there are still many questions with regard to the physics of the acceleration processes of these sources, and it is vital to understand in detail the dependence of the different acceleration mechanisms on the laser and target conditions” (Krushelnik et al., Reference Krushelnik, Clark, Beg, Dangor, Najmudin, Norreys, Wei and Zepf2005). This contribution presents some earlier results, yet unpublished (in this form, at least), and more recent ones that are concentrated mainly on the angular distribution of emitted ions and on the influence of the target irradiation angle.
EXPERIMENTAL ARRANGEMENT
The Nd:YAG laser LAB 100 at INFN-LNS in Catania, with the nominal energy of 900 mJ in 9 ns pulse duration was used for experiments at low laser intensities (1010 W/cm2). With a lens of focal length f = 500 mm, the laser beam was focused onto a target of various elements located in the target chamber evacuated to ~10−7 mbar. The minimum focus diameter was below 1 mm. The position of target chamber flanges (17°, 30°, 43°, and 56°) with regard to the laser input window, together with the rotating movable target holder made the measuring of the angular distribution of an ion emission possible (Torrisi et al., Reference Torrisi, Ciavola, Gammino, Andò, Barnà, Láska and Krása2000, Reference Torrisi, Andò, Gammino, Krása and Láska2001a, Reference Torrisi, Andò, Ciavola, Gammino and Barnà2001b; Láska et al., Reference Láska, Krása, Pfeifer, Rohlena, Gammino, Torrisi, Andò and Ciavola2002b).
The laser intensities above 1016 W/cm2 were delivered onto the target by a high-power iodine laser system PALS (λ = 1.315 µm, EL ≤ 1 kJ, τ ≤ 350 ps, IL ≤ 6 × 1016 W/cm2, possible conversion to 2ω and 3ω) at the PALS Research Centre in Prague (Jungwirth et al., Reference Jungwirth, Cejnarová, Juha, Králiková, Krása, Krouský, Krupièková, Láska, Mašek, Mocek, Pfeifer, Präg, Renner, Rohlena, Rus, Skála, Straka and Ullschmied2001; Jungwirth, Reference Jungwirth2005). Solid targets were irradiated either perpendicularly or at 30° with respect to the target normal. The laser beam was focused with an aspheric lens (f = 627 mm for 1ω and f = 600 mm for 3ω) onto targets with a minimum focus spot diameter of ~70 µm. The ICs were positioned inside the target chamber (Wolowski et al., Reference Wolowski, Badziak, Boody, Hora, Hnatowicz, Jungwirth, Krása, Láska, Parys, Peøina, Pfeifer, Rohlena, Ryc, Ullschmied and Woryna2002a). The data obtained in earlier experiments, employing an iodine laser system PERUN (Láska et al., Reference Láska, Krása, Mašek, Pfeifer, Králiková, Mocek, Skála, Straka, Trenda, Rohlena, Woryna, Farny, Parys, Wolowski, Mroz, Shumshurov, Sharkov, Collier, Langbein and Haseroth1996), completed the new experimental data. The positions of output windows of the smaller PERUN chamber were located at 40° (IC), 60° (S1), and 90° (S2) with regard to the laser beam (Woryna et al., Reference Woryna, Parys, Wolowski, Krása, Láska, Králiková, Skála and Rohlena1999) as shown in Figure 1.
![](https://static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary-alt:20160629012400-54363-mediumThumb-S0263034608000591_fig1g.jpg?pub-status=live)
Fig. 1. Scheme of the PERUN target chamber (CH – Target Chamber, L – Focusing Lens, T – Target Holder, IEA, IC, S1, S2, S3 – ICs).
In addition, a picosecond (sub-nanosecond) Nd:glass laser at the Institute of Physics and Laser Microfusion in Warsaw (λ = 1.05 µm, E L ≤ 1 J, τ ≤ 1 ps, I L ≤ 1 × 1017 W/cm2 (Wolowski et al., Reference Wolowski, Badziak, Krása, Láska, Parys, Rohlena and Woryna2002b; Badziak et al., Reference Badziak, Hora, Woryna, Jablonski, Láska, Parys, Rohlena and Wolowski2003, Reference Badziak, Glowacz, Jablonski, Parys, Wolowski, Hora, Krása, Láska and Rohlena2004) was used for short pulse experiments. The laser beam was focused onto a target by a parabolic mirror with a small hole in its center. The advantage of this mirror is a possibility to irradiate the target and simultaneously to detect the emitted ions along the target normal.
The corpuscular diagnostics was based on the time-of-flight (TOF) method using various types of ICs and a cylindrical electrostatic ion energy analyzer (IEA) (Láska et al., Reference Láska, Krása, Mašek, Pfeifer, Králiková, Mocek, Skála, Straka, Trenda, Rohlena, Woryna, Farny, Parys, Wolowski, Mroz, Shumshurov, Sharkov, Collier, Langbein and Haseroth1996; Woryna et al., Reference Woryna, Parys, Wolowski and Mróz1996b; Wolowski et al., Reference Wolowski, Badziak, Boody, Hora, Hnatowicz, Jungwirth, Krása, Láska, Parys, Peøina, Pfeifer, Rohlena, Ryc, Ullschmied and Woryna2002a). Ions were detected in a far expansion zone (~1 m) where the three-body recombination collisions are negligible and the ion charge-states are “frozen” (Rohlena et al., Reference Rohlena, Králiková, Krása, Láska, Mašek, Pfeifer, Skála, Parys, Wolowski, Woryna, Farny, Mroz, Roudskoy, Shamaev, Sharkov, Shumshurov, Bryunetkin, Haseroth, Collier, Kuttenberger, Langbein and Kugker1996). It is worth remembering that the appropriate critical length L cr from the target was measured to be ~20 cm for the Cu ions produced by an excimer (XeCl) laser delivering low intensity (Lorusso et al., Reference Lorusso, Krása, Rohlena, Nassisi, Belloni and Doria2005), and it is shorter than 80 cm for iodine laser delivering intensities about 1014 W cm−2 (Krása et al., Reference Krása, Láska, Rohlena, Pfeifer, Skála, Králiková, Straka, Woryna and Wolowski1999). However, it was calculated to be even longer than 1 m for CO2 laser (Roudskoy, Reference Roudskoy1996). A quadruple mass analyzer Quadstar 421 was used to investigate neutral species ejected from the target (Torrisi et al., Reference Torrisi, Ciavola, Gammino, Andò, Barnà, Láska and Krása2000, Reference Torrisi, Andò, Gammino, Krása and Láska2001a).
RESULTS AND DISCUSSION
Ions Produced at Low Laser Intensity
The laser beam, which is focused onto solid targets at low intensities, heats, melts, and evaporates the target material. Starting from some threshold intensity (~109 W/cm2 for Nd:YAG), the ions in addition to a different kind of neutrals are emitted. The threshold laser energies and the laser energy fluences for the ion generation of various target elements (Al, Au, Cu, Nb, Ni, Pb, Sn, Ta, W) were investigated (Torrisi et al., Reference Torrisi, Ciavola, Gammino, Andò, Barnà, Láska and Krása2000, Reference Torrisi, Andò, Gammino, Krása and Láska2001a, Reference Torrisi, Andò, Ciavola, Gammino and Barnà2001b). They are presented in Table 1 together with typical mean values of the velocity and kinetic energy of ions, corresponding to the ion current peaks, observed close to threshold intensities. The ion current densities were obtained using the relation:
![\,j={U \over R S T \lpar 1+ \gamma z\rpar },\eqno\lpar 1\rpar](https://static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20160126040956937-0419:S0263034608000591_eqn1.gif?pub-status=live)
U is the output IC voltage, the load resistance R = 25 Ω, S is the IC area, T is the IC grid transmission, γ is the coefficient of secondary electron emission induced by the impact of ions on the IC electrode, and z is the charge-state of ions. Melting points and boiling points of tested elements are included in Table 1 for completeness.
Table 1. Some typical characteristics of the tested elements and of the generated ions
![](https://static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20160126040956937-0419:S0263034608000591_tab1.gif?pub-status=live)
The angular distribution of ions produced by 9-ns pulses of the Nd:YAG laser was assembled from values of peak ion-current densities (1) measured simultaneously in four positions of ICs and changing stepwise the target tilt angle from 10° to 69° with regard to the laser beam. The peak ion currents were normalized to the peak current observed along the target surface normal. In fact, we obtained four dependencies, differing in laser irradiation angle (17°, 30°, 43°, 56°), as well as shifted with regard to each other in the region of the recorded distribution angles. This variation in the target tilt angle θ also results in a decrease of the irradiating laser intensity according to cosθ. The angular distributions of peak ion currents, obtained at laser intensities of about 5 × 109 W/cm2, are shown in Figures 2a–2i together with the fitted function
![j_{BL} +\, j_{\max} {\rm cox}^{p} \lpar \varphi - \varphi_{0} \rpar, \eqno \lpar 2 \rpar](https://static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20160126040956937-0419:S0263034608000591_eqn2.gif?pub-status=live)
where jBL is the base line of the measured TOF spectra j φ(t), j max is the peak value of j φ(t), and φ0 is the deviation from the target normal along with the main part of ions expands into the vacuum, as it is generally observed (Ehler, Reference Ehler1975). The shape of the angular distribution of ions was found to be independent of the angle of irradiation of the target up to 60°, in fact.
![](https://static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary-alt:20160629012504-47175-mediumThumb-S0263034608000591_fig2g.jpg?pub-status=live)
Fig. 2. Angular distributions of normalized current densities of emitted ions, jN, produced by low laser-intensities, irradiating various target elements (for more details, see text).
The fitted values of the exponent p and the corresponding widths (full width at half maximum, FWHM) of the measured angular distributions of ion currents shown in Figure 2 are the content of Table 1. The phenomenological description of the angular dependence of the peak ion-current is improved generally by an extension of Eq. 2 to a 0 + a 1 cos(ϕ – ϕ0) + a p cosp(ϕ – ϕ0) – (two component structure) (Thum et al., Reference Thum, Rupp and Rohr1994; Woryna et al., Reference Woryna, Badziak, Krasa, Laska, Makowski, Parys, Rohlena, Vankov and Wolowski2001). According to Buttini et al. (Reference Buttini, Thum-Jager and Rohr1998) and Thum-Jager and Rohr (Reference Thum-Jager and Rohr1999), the exponent p should increase and FWHM should decrease with the increasing ion mass, A, approximately following A1/2 or A3/4 law, as it was observed for the total charge emitted or the numbers of particular ion species, respectively. However, these atomic mass dependencies of the angular distribution observed for the peak ion-currents were not found completely confirmed. The broadest angular distribution of an ion current was observed for Al, the narrowest one for W.
Some additional questions are evoked in connection with the angular distribution of ions: what is the kind, number, and energy of single ions, emitted into different (chosen) angles with regard to the target normal (isotropy of ion-carried kinetic energy), and whether there are any differences and which one in ion characteristics, comparing ion expansion against (−) or in the direction (+) of radiation of the laser beam. The IC gives the time-resolved, but charge-integrated signal, U(t) = R i(t) = R dQ/dt = R d(N(t) <z(t)> e)/dt, where N(t) is the number of ions, <z(t)> is the averaged charge-state of ions at the instant t, and e is the elementary charge. Since the measured ion current is a sum of particular currents of various ionized species, both magnitudes N and <z> must be determined with the use of another kind of ion diagnostics such as a cylindrical IEA or Thomson parabola spectrograph (TPS) (Woryna et al., Reference Woryna, Parys, Wolowski and Mróz1996b), or the diagnostics can be completed by a numerical deconvolution of IC signal with more or less peaks or humps (Krása et al., Reference Krása, Jungwirth, Krouský, Láska, Rohlena, Pfeifer, Ullschmied and Velyhan2007; Picciotto et al., Reference Picciotto, Krása, Láska, Rohlena, Torrisi, Gammino, Mezzasalma and Caridi2006). The retrieval of the particular ion currents, produced by various mechanisms, makes the determination of the total number N of ions and their mean charge state <z> possible. Then the integral of an IC signal, i.e., the value of the total charge of collected ions can be interpreted in the frame of the product N <z> e. Similarly, it is possible to determine experimentally the mean velocity <v i> and the total energy of expanding ions E = <E i > N, where <E i> is the mean energy carried by a single ion. This simplest analysis of IC signals measured at different directions of the plasma expansion can contribute to elucidation of the phenomenological angular dependence represented by Eq. (2) or its expanded version. It is evident that the angular expansion of the plasma depends not only on the hydrodynamic properties of the plasma but also on the created ambipolar electric field, accelerating the ions mainly along the target normal (Krása et al., Reference Krása, Jungwirth, Krouský, Láska, Rohlena, Pfeifer, Ullschmied and Velyhan2007). Therefore, the above-mentioned effect of the ion mass on the value of FWHM should be completed by the angular distribution of centre-of-mass velocity of particular ion species.
The expansion of laser-produced plasma primarily depends on the velocity distribution of the expanding ion species (Stritzker et al., Reference Stritzker, Pospieszczyk and Tagle1981; Kelly & Dreyfus, Reference Kelly and Dreyfus1988). As it was presented elsewhere (Krása et al., Reference Krása, Jungwirth, Krouský, Láska, Rohlena, Ullschmied and Velyhan2008), the response of IC to an impacting ion current can be expressed in the form
![\,j_{IC} \lpar t\rpar \propto v_{x} \,f\lpar \vec {v}\rpar d\vec {v} \propto {L^{2} \over t^{5}} f \left({L \over t}\right)\comma \; \eqno\lpar 3\rpar](https://static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20160126040956937-0419:S0263034608000591_eqn3.gif?pub-status=live)
where f is the velocity distribution, t is the TOF through the distance L. If a shifted Maxwell–Boltzmann velocity distribution describes the properties of the expanding fluid, then the IC signal is
![\,j_{IC} \lpar L\comma \; t\rpar \propto t^{-5} \hbox{exp}\lsqb \!-\!\beta^{2} \lpar L/t - u\rpar ^{2}\rsqb \comma \; \eqno\lpar 4\rpar](https://static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20160126040956937-0419:S0263034608000591_eqn4.gif?pub-status=live)
where β2 = m i/2kT, and u is the center-of-mass velocity. The peak velocity, i.e., the velocity corresponding to the maximum of a time-resolved ion current (TOF spectrum), is expressed by:
![u_{\,peak} = {1 \over 5} \sqrt {m \over 2kT} \left(\sqrt {10 + {m u^{2} \over 2kT}} - \sqrt {m u^{2} \over 2kT}\right).\eqno\lpar 5\rpar](https://static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20160126040956937-0419:S0263034608000591_eqn5.gif?pub-status=live)
Since the ion current detected with an IC is composed of particular currents j A,q of a number of ion species having atomic mass A and charge-state q
![\,j_{IC} \lpar L\comma \; t\rpar = \sum_{A\comma q} j_{A\comma q} \lpar L\comma \; t\rpar \eqno\lpar 6\rpar](https://static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary:20160126040956937-0419:S0263034608000591_eqn6.gif?pub-status=live)
Eq. (3) should be substituted in Eq. (5). Then the equation expressing the peak velocity of the total current would depend on the number of parameters relating to all the particular currents as the numbers of ion species, their center-of-mass velocities and the temperature. For simplicity Eq. (4) could help to elucidate the angular dependencies of peak velocities (energies) measured for various elements shown in Figure 3.
![](https://static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary-alt:20160629012804-87111-mediumThumb-S0263034608000591_fig3g.jpg?pub-status=live)
Fig. 3. (Color online) Angular distributions of the peak (mean) ion velocity <v> (with respect to the target normal and corresponding to the Fig. 2).
The center-of-mass velocity u, which is generally dependent on the accelerating ambipolar field and collisional rates of ions, significantly affects the peak velocity, as Eq. (4) suggests (Krása et al., Reference Krása, Jungwirth, Krouský, Láska, Rohlena, Pfeifer, Ullschmied and Velyhan2007). If the laser beam hits a target obliquely, then the plasma expanding along the target normal could interact with the laser beam only by its lateral part. Such interaction could result in acceleration of fast electrons along the laser-beam axis with a consequent increase in center-of-mass velocity u in the range of angle from −10° to −69°, as the target is rotated. The highest asymmetry in the angular distribution of peak velocities shows the Au-plasma (Fig. 3a). The maximum near the target normal, i.e., at 0°, was well distinguishable for Nb-, W-, Cu- and Al-plasmas, as Figures 3b to 3e show. The peak velocity of expanding Ni- and Ta-plasmas are nearly angular independent, see Figures 3f and 3g. A more complex dependence (decrease) in the peak velocity was observed for Pb- and Sn-plasmas, but a peak-velocity enhancement at about 30° can be hardly elucidated without invoking a formation of side jet-like plasma emission during the plasma production. For the precise description of this phenomenon, it would be necessary to determine the particular currents of all the emitted ion species or to retrieve these particular currents by a mathematical deconvolution method of IC signal, i.e., TOF spectrum, based on Eqs. (3) and (5) (Krása et al., Reference Krása, Jungwirth, Krouský, Láska, Rohlena, Pfeifer, Ullschmied and Velyhan2007, Reference Krása, Jungwirth, Krouský, Láska, Rohlena, Ullschmied and Velyhan2008).
It is worth remembering at this moment that the IC signal reflects the plasma production mechanisms, participating in the ion production (Láska et al., Reference Láska, Jungwirth, Krása, Pfeifer, Rohlena, Ullschmied, Badziak, Parys, Wolowski, Gammino, Torrisi and Boody2005a, Reference Láska, Jungwirth, Krása, Pfeifer, Rohlena and Ullschmied2005b), and also influencing the direction of the ion expansion. The planar geometry of the target tends to emit ions due to the strong ambipolar electric field accelerating the ions perpendicularly to the target, while the radial component of the ponderomotive or thermo-kinetic forces drive them radially with regard to the laser beam axis.
Ions Produced by High Laser Intensity
Starting from the laser intensity of ~1014 W/cm2, non-linear processes in the pre-formed (pre-pulse) plasma support the generation of ions with the highest energy and the highest charge states (Láska et al., Reference Láska, Jungwirth, Králiková, Krása, Pfeifer, Rohlena, Skála, Ullschmied, Badziak, Parys, Wolowski, Woryna, Torrisi, Gammino and Boody2004a, Reference Láska, Jungwirth, Krása, Pfeifer, Rohlena, Ullschmied, Badziak, Parys, Wolowski, Gammino, Torrisi and Boody2005a; Badziak et al., Reference Badziak, Kasperczuk, Parys, Pisarczyk, Rosinski, Ryć, Wolowski, Jablonski, Suchanska, Krouský, Láska, Mašek, Pfeifer, Ullschmied, Dareshwar, Foldes, Torrisi and Pisarczyk2007) (see Fig. 4). Also experiments of VanRompay et al. (Reference Vanrompay, Nantel and Pronko1998) with the fs laser (1015 W/cm2) and carbon target confirmed that the size, shape, and charge states of the ion energy distributions in the ablation plume depend strongly on the laser intensity, and even more importantly, on the laser pulse contrast. The presence of pre-pulse can significantly modify this distribution.
![](https://static.cambridge.org/binary/version/id/urn:cambridge.org:id:binary-alt:20160629013129-24321-mediumThumb-S0263034608000591_fig4g.jpg?pub-status=live)
Fig. 4. Highly charged Au and Pb ions recorded by IEA (Au: 1ω, E L = 14.5 J, ϕ = 25°, FP = −125 µm, E/z = 20 keV; Pb: 1ω, E L = 22.7 J, ϕ = 35°, FP = −100 µm, E/z = 20 keV).
If ions with a high energy (~1 MeV) are generated in the laser plasma, directional maxima of ion emission other than normally to the target may appear in addition to the main ion peak. High-energy (0.15–4 MeV) fast phosphor ions produced at laser power densities ~1015 W/cm2, were found to be emitted almost parallel to the target surface by Basov et al. (Reference Basov, Getz, Maksimchouk, Mikhailov, Rode, Sklizkov, Fedotov, Ferster and Hora1987). This fact was explained by the acceleration of ions due to the ponderomotive forces at relativistic self-focusing of the laser beam in the plasma (Hora, Reference Hora1975; Hauser et al., Reference Hauser, Scheid and Hora1992). We observed a second maximum for Al ion velocities from 1 × 107 cm/s to 1 × 108 cm/s (energy up to 140 keV) at about 60° from the target normal (Chvojka et al., Reference Chvojka, Králiková, Krása, Láska, Mašek, Rohlena, Skála, Mroz, Parys, Wolowski and Woryna1994; Mróz et al., Reference Mróz, Parys, Wolowski, Woryna, Králiková, Krása, Láska, Mašek, Skála and Rohlena1994). (If the angular distribution is presented in the polar coordinates, an approximate form of expanding plasma plume is recovered due to the point-like source of ions.)
The PERUN laser (5 × 1014 W/cm2) was used for more detailed studies of angular distribution of the emitted Au, Pb, and Sn ions (Woryna et al., Reference Woryna, Parys, Wolowski, Krása, Láska, Králiková, Skála and Rohlena1999). IC signals, measured at various angles, were normalized to the same distance of 144 cm according to the j ~ L IC−3 law. The velocity limit of 1 × 108 cm/s was postulated to define the slow and the fast ions. This separation also helps to determine the charge carried by both the ion groups. The IC signals were integrated over two TOF ranges, corresponding to the separate two ion groups mentioned. Figure 5 shows an example of the angular distribution of the charge density of the slow (energy lower than ~1 MeV, broken line) and fast (energy higher than ~1 MeV, full thin line) Au ion groups, determined in the above-mentioned way. The thick full line represents angular distribution of the total charge density, which is a sum of the partial distributions of both ion groups. In this case, the FP = −125 µm was in front of the target surface, and the target tilt angle ϕ was 40°. The preferred emission angle of slow ions is close to the target normal (about 40° to the laser beam), while it is about 20° with respect to the target normal (i.e., about 60° to the laser beam) for the fast ions. Preferred direction (angle) of total charge (the sum of both slow and fast groups) is within about 10° from the target normal (about 50° to the laser beam axis). Changing the target tilt angle from 20° to 45°, the preferred direction of emission of the slow ion group remains close to the target normal, while for the fast ion group the preferred emission angle decreases from ~40° to ~20° with respect to the target normal. Figure 6 shows an angular distribution of the total charge density of Au and Pb ions at various angles of target irradiation (tilt angle 20°–45°, see symbol labels in Fig. 6) and related to the IC position (40°). Considering the preferred emission angles of the total charge of both ion groups, they reflect the number (ratio) of the produced slow and fast ions, and, in fact, also a kind of prevailing mechanism of their generation and acceleration. The dependence of preferred emission angles of total ion charge on the target tilt angle is shown in Figure 7. However, the situation is more complex due to the dependence on laser FP, which significantly affects the ion production independently of the irradiation angle. This fact is clearly demonstrated for Au and Sn ions in Figure 8.
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Fig. 5. Angular distribution of the charge density of slow (thin dotted line) and fast (thin full line) Au ions and of the total charge density (thick full line); 1ω, E L = 30 J, ϕ = 40°, FP = −125 µm (for more details, see text).
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Fig. 6. (Color online) Angular distribution of the total charge density, Q, of Au (a) and Pb (b) ions at target tilt angles 20°–45° (Au: 3ω, E L = 30 J, FP = −125 µm. Pb: 3ω, E L = 22 J, FP = −20 µm).
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Fig. 7. (Color online) Preferred emission angles of the total charge, Q, of Au and Pb ions in dependence on the target tilt (irradiation) angle (Au: 3ω, E L = 30 J, FP = −125 µm. Pb: 3ω, E L = 22 J, FP = −20 µm).
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Fig. 8. (Color online) Preferred emission angles of the total charge, Q, of Au and Pb ions in dependence on the FP at fixed laser energy and irradiation angle (Au: 3ω, E L = 19 J, ϕ = 30°. sn: 3ω, E L= 24 J, ϕ = 40°).
Values of ion charge states up to ~57+ and peak ion energy ~30 MeV for Au and Ta ions were recorded by using the PALS laser system at intensities up to 5 × 1016 W/cm2. The higher laser intensity, the larger preferred emission angle of the fast ion groups. Angular distributions of emitted Ta ions presented in Figure 9, all produced at laser frequency 3ω, were determined with ICs located inside the target chamber (Badziak et al., Reference Badziak, Glowacz, Jablonski, Parys, Wolowski, Hora, Krása, Láska and Rohlena2004; Wolowski et al., Reference Wolowski, Badziak, Boody, Gammino, Hora, Jungwirth, Krása, Láska, Parys, Pfeifer, Rohlena, Szydlowski, Torrisi, Ullschmied and Woryna2003, Reference Wolowski, Badziak, Boody, Czarnecka, Gammino, Jablonski, Krása, Láska, Parys, Rohlena, Rosinski, Ryc, Torrisi and Ullschmied2006) at short distances of ~50 cm from the target. Lower ion current densities (curve 1) were recorded at a target tilt (irradiation) angle of ϕ = 30° (E L = 225 J). Higher ion currents (curve 2) were measured at the perpendicular target irradiation (ϕ = 0°), in this case, E L = 140 J only. The highest ion yield (curve 3) was recorded with the separate laser pre-pulse (~10 J) 4.6 ns before the main pulse, at the same other experimental conditions. Significant effect of interaction of laser beam with the pre-formed plasma was also confirmed in different sns-pulse experiments by finding preferred emission maxima for Au ions at ~24o, not perpendicular to the target surface (see Fig. 10). Angular distribution for ps pulse is included for a comparison (Wolowski et al., Reference Wolowski, Badziak, Krása, Láska, Parys, Rohlena and Woryna2002b; Badziak et al., Reference Badziak, Hora, Woryna, Jablonski, Láska, Parys, Rohlena and Wolowski2003, Reference Badziak, Glowacz, Jablonski, Parys, Wolowski, Hora, Krása, Láska and Rohlena2004).
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Fig. 9. (Color online) Angular distribution of the maximum at current density of Ta ions, j max, recorded at high laser intensities (PALS) At three various irradiation conditions (1 – 3ω, E L = 225 J, ϕ = 30°, FP = 0 µm; 2−3ω, E L = 140 J, ϕ = 0°, FP = 0 µm; 3−3ω, E L = 140 J, ϕ = 0°, FP = 0, 10 J pre-pulse 4.6 ns before the main pulse).
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Fig. 10. (Color online) Angular distribution laser of the maximum current density of Au ions, j max, produced by Nd:YAG laser, delivering picosecond (ps) and sub-nanosecond (s-ns) pulses at high intensities (ps1 – E L = 0.52 J, τ = 1 ps, ϕ = 0°, FP = 0 µm; sns1 – E L = 0.56 J, τ = 0.5 ns, ϕ = 0°, FP = 0 µm; sns2 – E L = 0.49 J, τ = 0.5 ns, ϕ = 0°, FP = −400 µm).
The main part of the emitted ions in most of the experiments is reported along the target normal. This fact corresponds also to the results of systematic interferometric studies of plasma jets, emitted from the plasma of various target elements (Al, Au, Cu, Pb, Ta) (Schaumann et al., Reference Schaumann, Schollmeier, Rodriguez-Prieto, Blazevic, Brambrink, Geissel, Korostiy, Pirzadeh, Roth, Rosmej, Faenov, Pikuz, Tsigutkin, Maron, Tahir and Hoffmann2005; Nicolai et al., Reference Nicolaï, Tikhonchuk, Kasperczuk, Pisarczyk, Borodziuk, Rohlena and Ullschmied2006; Kasperczuk et al., Reference Kasperczuk, Pisarczyk, Borodziuk, Ullschmied, Krousky, Masek, Rohlena, Skala and Hora2006, Reference Kasperczuk, Pisarczyk, Borodziuk, Ullschmied, Krousky, Masek, Pfeifer, Rohlena, Skala and Pisarczyk2007). Such plasma jets are about 200 µm in diameter (very similar for each element), about 3 mm long, and with a surprisingly high lifetime measured up to ~20 ns, at least. However, it does not mean that these ions must be the fastest one. Some available interferogram pictures suggest the existence of two additional side groups of ions with the preferred directions ± ~40° with regard to the target normal, the parameters of which may be even higher.
CONCLUSION
Generally, it is accepted that the majority of ions from laser-produced plasma is emitted along the target normal. This is based on the planar target, the geometry of which tends to form narrow jets of high-energy ions with the high charge states. However, more detailed systematic measurements proved that especially at high laser power densities and with the significant participation of non-linear processes, other preferred directions or smaller secondary maxima can appear. A very important role is played by the laser beam interaction with pre-formed laser plasma, as well as the focus setting, and the angle of irradiation of target surface, especially at high laser intensities. Planar geometry of the target tends to prefer the emission (acceleration) of ions perpendicularly to the target due to the ambipolar electric field of escaping thermal or fast electrons, while the radial component of the ponderomotive or thermo-kinetic forces drives them radially with regard to the laser beam axis.
ACKNOWLEDGMENT
This contribution is dedicated to the memory of our colleague E. Woryna who started this work a few years ago, but he did not manage to finish it. M. Lásková is acknowledged for the technical help. The grant agency of the Academy of Sciences of the Czech Republic kindly supported this work (project number IAA 100100715). The support of the 5th National Committee of INFN to the platone experiment is also acknowledged.